Cyanogen Imaging® MaxIm DLTM 包含一套全面的图像采集、处理和分析工具。从完整的天文台集成开始，MaxIm DL 可帮助您轻松完成从原始数据收集到最终高质量结果的整个过程。
文件大小：187.1 MB
Cyanogen Imaging® MaxIm DLTM 提供涵盖图像获取、处理及分析的完整工具套件。通过全面整合天文台设备，该软件能以迷你动画工作量引导用户完成从原始数据采集到生成高质量成果的全流程。
典型成像序列支持包含数小时的抖动自动导引曝光、自动滤光片切换及赤道仪翻转操作——同时可控制圆顶随动并实时监测气象数据。每个图像的FITS头文件均包含丰富元数据标注。当气象传感器检测到危险条件时，软件将自动关闭设备、归位望远镜并锁定圆顶。
完成图像采集后，软件可自动分类校准帧组并为每帧图像匹配最佳校准组，实现快速校准与堆栈处理。通过简单点击即可批量处理不同目标的数百幅图像。
该软件集专业级测光与天体测量功能于一体：测光采用经天文学家认证的中值平均算法与亚像素分割技术；天体测量则搭载当前公认最精准强大的PinPoint LE模块。
核心特性
完整天文台集成方案，全面控制天文设备
支持相机、导星设备、滤光轮、调焦器、相机旋转器、赤道仪、监控摄像头、继电器、气象站及圆顶的集成操控
完全兼容ASCOM协议
内置迷你天象仪增强操作环境感知
高效预设功能，自定义寻星-居中-对焦-成像序列
多线程硬件接口确保流畅响应
用户自定义条件触发器（含气象模块）实现自动关停
PinPoint V6实时全天解析，快速定位丢失目标
导星重捕获赤道仪自动翻转
多星差分导引技术
通过监控摄像、远程开关及气象监测实现天文台管控
批量堆叠多目标图像，支持自动对齐与异常帧剔除
窄带数据融合生成真实影像或伪彩色渲染
完整图像处理工具包涵盖：多元滤镜、消星芒、曲线调整、反卷积算法及色彩工具等
海量多光谱测光数据分析，支持光变曲线导出与AAVSO报告生成
RAW文件即时彩色预览（无需拜耳转换）
Cyanogen Imaging® MaxIm DLTM 包含一套全面的图像采集、处理和分析工具。从完整的天文台集成开始，MaxIm DL 可帮助您轻松完成从原始数据收集到最终高质量结果的整个过程。
File size: 187.1 MB
Cyanogen Imaging® MaxIm DLTM includes an extensive suite of image acquisition, processing, and analysis tools. Starting with complete observatory integration, MaxIm DL takes you from gathering raw data through to the final high-quality result with the minimum of effort.
A typical imaging sequence will include hours of autoguided images with dither, automatic filter changes, and pier flipping – all the while slewing your dome and monitoring the weather. Every image is tagged with extensive data in its FITS header. When your weather sensor reports unsafe conditions MaxIm DL will automatically shut down your equipment, park the telescope, and safe the dome.
Once your images are collected, MaxIm DL can automatically assemble your calibration images into groups, select the correct groups for each individual image, calibrate, and stack your images. You can process hundreds of images from different targets with just a few mouse clicks.
MaxIm DL also includes advanced photometry and astrometry capabilities. Photometric measurements are made using best practice median-mean and partial-pixel algorithms vetted by professional astronomers. Astrometric measurements are performed using PinPoint LE, widely recognized as the most powerful and accurate package available today.
Key 资源特色
Complete observatory integration. Controls all of your astronomical equipment.
Integrates your camera, autoguider, filter wheels, focusers, camera rotator, telescope mount, observatory webcam, remote switches, weather station, and dome.
Fully ASCOM compliant.
Built-in mini-planetarium helps you maintain “situational awareness”.
Designed for efficiency. Create your own presets for finding, centering, focusing, and imaging sequences.
Multithreaded hardware interfaces for smooth and responsive operation.
Automated shutdown with user-definable triggers (including weather) and sequencing.
PinPoint V6 with online all-sky solving – easily recover if your telescope gets lost.
Automatic pier flipping with guide star reaquisition.
Multistar and differential autoguiding.
Monitor and control your observatory with dome webcam, remote switches, and weather monitoring.
Stack hundreds of images of different targets in one operation – with automatic alignment and bad data rejection.
Blend in narrowband data to create fully realistic images or false color representations of your data.
Includes a complete image processing toolkit, including a large variety of filters, deblooming, curves, deconvolution, color tools, and much more.
Analyze multispectral photometry data for huge numbers of images including multiple targets; export light curves and AAVSO reports.
Instant Raw image color preview – see Raw images in full color without Bayer conversion.
